Search results for "Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik"

showing 10 items of 223 documents

Measurement of ultra-low heating rates of a single antiproton in a cryogenic Penning trap

2019

Physical review letters 122(4), 043201 (2019). doi:10.1103/PhysRevLett.122.043201

Electric fieldsField noiseCryogenicsAtomic Physics (physics.atom-ph)Penning trapOther Fields of PhysicsGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences530physics.atom-phPhysics - Atomic PhysicsSpectral densityNoise spectral densityTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530010306 general physicsPhysicsComputer Science::Information RetrievalSpectral densityComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)Penning trapOrders of magnitudeAntiprotonQuantum transition rateDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikAtomic physicsPräzisionsexperimente - Abteilung BlaumIon traps
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Experimental investigation of low-frequency pulsed Lorentz force influence on the motion of Galinstan melt

2016

Abstract The paper presents the results of the numerical and physical experiments, aimed at assessing the influence of pulsed force of electromagnetic field on the melt motion and the fluid velocities. The experiment was performed on the eutectic alloy Galinstan in the cylindrical volume, where an ultrasonic Doppler velocimeter was employed for velocity measurements under conditions of pulsed and steady EM field application. A numerical simulation of the melt flow, forced by the steady EM force, involved a 2D axisymmetric model. The k-e turbulence model was used to obtain the information about the melt velocities. The verification of the numerical model was carried out for the steady case. …

Electromagnetic field02 engineering and technologyLow frequency01 natural sciencesElectromagnetic stirring020501 mining & metallurgy010305 fluids & plasmasNuclear magnetic resonancesymbols.namesakechemistry.chemical_compoundLorentz forceOptics0103 physical sciencesElectromagnetic fieldddc:530Modulated Lorentz forceClassical mechanicsddc:510Mathematical PhysicsMelt flow indexPhysicsComputer simulationTurbulencebusiness.industryPhysicsStatistical and Nonlinear PhysicsMechanicsPulsedCondensed Matter PhysicsDoppler effectGalinstanDewey Decimal Classification::500 | Naturwissenschaften::510 | MathematikAtomic and Molecular Physics and OpticsGalinstanTurbulenceEutectic system0205 materials engineeringchemistrysymbolsDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikbusinessLow frequencyMelt flow indexDoppler effectLorentz forceMathematical simulationSt. Petersburg Polytechnical University Journal: Physics and Mathematics
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Influence of the channel design on the heat and mass exchange of induction channel furnace

2011

PurposeThe purpose of this paper is to present in‐depth numerical modelling of heat and mass exchange in industrial induction channel furnace (ICF).Design/methodology/approachThe turbulent heat and mass exchange in the melt is calculated using a three‐dimensional (3D) electromagnetic model and a 3D transient large eddy simulation method. The simulation model has been verified by flow velocity and temperature measurements, which were carried out using an industrial sized channel inductor operating with Wood's metal as a low temperature model melt.FindingsThe ICF is well‐established for melting, holding and casting in the metallurgical industry. But there are still open questions regarding th…

EngineeringElectromagnetic modelsLarge Eddy simulation methodsChannel geometryHeat and mass transferDewey Decimal Classification::600 | Technik::620 | Ingenieurwissenschaften und MaschinenbauMechanical engineeringInductorTemperature measurementModellingMetallurgical industryChannel designExperimentWood's metalMass transferLow temperaturesIndustryMass transferWood's metalElectrical and Electronic Engineeringddc:510Low frequency oscillationsMass exchangeTemperature measurementbusiness.industryApplied MathematicsThree dimensionalFurnaceMechanicsDesign/methodology/approachDewey Decimal Classification::500 | Naturwissenschaften::510 | MathematikComputer Science ApplicationsComputational Theory and MathematicsFlow velocityThree-dimensional (3D)Casting (metalworking)Numerical modellingMetallurgySimulation modelddc:620businessSimulationCommunication channelLarge eddy simulationNumerical analysis
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Numerical studies of the melting process in the induction furnace with cold crucible

2008

PurposeAims to present recent activities in numerical modeling of cold crucible melting process.Design/methodology/approach3D numerical analysis was used for electromagnetic problem and 3D large eddy simulation (LES) method was applied for fluid flow modeling.FindingsThe comparative modeling shows, that higher H/D ratio of the melt is more efficient when total power consumption is considered, but this advantage is held back by higher heat losses through the crucible walls. Also, calculations reveal that lower frequencies, which are energetically less effective, provide better mixing of the melt.Originality/value3D electromagnetic model, which allows to take into account non‐symmetrical dist…

EngineeringFurnacesMixing (process engineering)Dewey Decimal Classification::600 | Technik::620 | Ingenieurwissenschaften und MaschinenbauThermodynamicsCrucibleInduction furnaceElectromagnetic problemsModellingPhysics::Fluid DynamicsElectromagnetismElectromagnetismFluid dynamicsddc:510Electrical and Electronic Engineeringbusiness.industryApplied MathematicsNumerical analysisLarge eddy simulationMechanicsMeltingCold crucibleDewey Decimal Classification::500 | Naturwissenschaften::510 | MathematikComputer Science ApplicationsComputational Theory and MathematicsCruciblesddc:620Joule heatingbusinessSimulationLarge eddy simulationNumerical analysis
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Interaction-induced spin polarization in quantum dots.

2010

The electronic states of lateral many electron quantum dots in high magnetic fields are analyzed in terms of energy and spin. In a regime with two Landau levels in the dot, several Coulomb blockade peaks are measured. A zig-zag pattern is found as it is known from the Fock-Darwin spectrum. However, only data from Landau level 0 show the typical spin-induced bimodality, whereas features from Landau level 1 cannot be explained with the Fock-Darwin picture. Instead, by including the interaction effects within spin-density-functional theory a good agreement between experiment and theory is obtained. The absence of bimodality on Landau level 1 is found to be due to strong spin polarization.

Fock-Darwin spectrumSpin polarizationSpin-density-functional theoryQuantum DotGeneral Physics and AstronomyFOS: Physical sciencesElectronSpin dynamicsShubnikov–de Haas effectMesoscale and Nanoscale Physics (cond-mat.mes-hall)Electronic statesSemiconductor quantum dotsddc:530Landau levelsSpin-½PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsSpin polarizationCoulomb blockadeHigh magnetic fieldsLandau quantizationCondensed Matter::Mesoscopic Systems and Quantum Hall EffectMagnetic fieldQuantum dotMagnetic fieldsDensity functional theoryDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikInteraction effectPhysical review letters
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A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo

2021

This paper presents the gravitational-wave measurement of the Hubble constant (H 0) using the detections from the first and second observing runs of the Advanced LIGO and Virgo detector network. The presence of the transient electromagnetic counterpart of the binary neutron star GW170817 led to the first standard-siren measurement of H 0. Here we additionally use binary black hole detections in conjunction with galaxy catalogs and report a joint measurement. Our updated measurement is H 0 = km s-1 Mpc-1 (68.3% of the highest density posterior interval with a flat-in-log prior) which is an improvement by a factor of 1.04 (about 4%) over the GW170817-only value of km s-1 Mpc-1. A significant …

Gravitacióneutron star: binarycosmological model010504 meteorology & atmospheric sciencesAstronomyGravitational Waves Hubble constant O2 LIGO Virgodetector: network01 natural sciencesCosmologyGeneral Relativity and Quantum CosmologyLIGOdark energy010303 astronomy & astrophysicsQCPhysicsSettore FIS/01Hubble constantSettore FIS/05CATALOGPhysical Sciencessymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)DATA RELEASECOSMOLOGICAL PARAMETERSFOS: Physical sciencesO2General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsLUMINOSITY FUNCTIONSgravitational radiation: direct detectionGravitational-wave astronomy1STArticleelectromagnetic field: productionsymbols.namesakeBinary black hole0103 physical sciencesDISTRIBUTIONS/dk/atira/pure/subjectarea/asjc/1900/1912K-CORRECTIONSSDG 7 - Affordable and Clean EnergyAstrophysiqueSTFC0105 earth and related environmental sciencesGravitational Waves/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyScience & TechnologyGravitational waveVirgoAstronomyRCUKAstronomy and Astrophysicscosmology; gravitational waves; Hubble constant310 Galaxies and CosmologyLIGOGalaxyEVOLUTIONDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiegravitational radiation detectorVIRGOblack hole: binarySpace and Planetary Science[SDU]Sciences of the Universe [physics]DENSITYgravitational radiation: emissionDark energyAstronomiaddc:520/dk/atira/pure/subjectarea/asjc/3100/3103galaxyGravitational wave astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Hubble's lawThe Astrophysical Journal
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Soldner, Einstein, gravitational light deflection and factors of two

2021

GravitationPhysicssymbols.namesakeClassical mechanics510 MathematicsDeflection (physics)General relativity530 PhysicssymbolsGeneral Physics and Astronomy510 MathematikEinstein530 Physik
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First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

2017

Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors. In the case of known pulsars a fully coherent search, based on matched filtering, which uses the position and rotational parameters obtained from electromagnetic observations, can be carried out. Matched filtering maximizes the signal-to-noise (SNR) ratio, but a large sensitivity loss is expected in case of even a very small mismatch between the assumed and the true signal parameters. For this reason, {\it narrow-band} analyses methods have been developed, allowing a fully coherent search for gravitational waves from known …

Gravitational-wave observatoryPhysics and Astronomy (miscellaneous)Astronomy01 natural sciencesrotationneutron starsGeneral Relativity and Quantum Cosmologygravitational waves; LIGO; stochastic gravitational-waveLIGOneutron star010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCpulsarQBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Gravitational Waves neutron stars advanced detectors narrow-band searchDetectorAmplitude[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaasymmetryCoherence (physics)young pulsarinterferometerneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)proper motionadvanced detectorsGravitational wavesPulsar0103 physical sciencesddc:530Gravitational Waves010308 nuclear & particles physicsGravitational wavegravitational radiation530 PhysikLIGOgravitational radiation detectorComputational physicscoherencedetector: sensitivityNeutron starelectromagneticPhysics and AstronomyGravitational waves; Pulsarnarrow-band searchDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]discovery
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Can we fit nuclear PDFs with the high-x CLAS data?

2020

AbstractNuclear parton distribution functions (nuclear PDFs) are non-perturbative objects that encode the partonic behaviour of bound nucleons. To avoid potential higher-twist contributions, the data probing the high-x end of nuclear PDFs are sometimes left out from the global extractions despite their potential to constrain the fit parameters. In the present work we focus on the kinematic corner covered by the new high-x data measured by the CLAS/JLab collaboration. By using the Hessian re-weighting technique, we are able to quantitatively test the compatibility of these data with globally analyzed nuclear PDFs and explore the expected impact on the valence-quark distributions at high x. W…

Hessian matrixParticle physicsPhysics and Astronomy (miscellaneous)EMC effectNuclear TheoryFOS: Physical sciencesPartonlcsh:Astrophysicshiukkasfysiikka01 natural sciences114 Physical sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNuclear ExperimentEngineering (miscellaneous)Physics010308 nuclear & particles physicsddc:530530 Physiknuclear parton distribution functions (nuclear PDFs)High Energy Physics - PhenomenologyDistribution functionsymbolslcsh:QC770-798Nucleonydinfysiikka
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Aspects of chiral symmetry in QCD at T = 128 MeV

2023

We investigate several aspects of chiral symmetry in QCD at a temperature of $T = 128\,\text{MeV}$. The study is based on a $24\times 96^3$ lattice-QCD ensemble with O($a$)-improved Wilson quarks and physical up, down and strange quark masses. The pion quasiparticle turns out to be significantly lighter than the zero-temperature pion mass, even though the corresponding static correlation length is shorter. We perform a quantitative comparison of our findings to predictions of chiral perturbation theory. Among several order parameters for chiral symmetry restoration, we compute the difference of the vector- and axial-vector time-dependent correlators and find it to be reduced by a factor $\s…

High Energy Physics - Lattice530 PhysicsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesLattice QCD530 Physik
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